On the role of solar flare generated ions in producing high energy (> 300 keV) ion events upstream from the Earth's bow shock
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics
Reference8 articles.
1. Formation of shock-spike events at quasi-perpendicular shocks
2. Shock drift acceleration of energetic (E≥ 50 keV) protons and (E≥ 37 keV/n) alpha particles at the Earth’s bow shock as a source of the magnetosheath energetic ion events
Cited by 6 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Evidence and features of magnetospheric particle leakage on days 30–36, 1995: Wind, Geotail, and IMP 8 observations compared;Journal of Geophysical Research;2005
2. The spatial size of ion events measured far upstream of the Earth's bow shock by ACE/ULEIS and WIND/STEP;Geophysical Research Letters;2000-01-01
3. Characteristics of >= 290 keV magnetosheath ions;ANN GEOPHYS-ATM HYDR;1999
4. Comment on ‘Energetic heavy ions observed upstream of the Earth's bow shock by the STEP/EPACT instrument on WIND’ by G. M. Mason, J. E. Mazur, and T. T. Von Rosenvinge;Geophysical Research Letters;1998-05-01
5. Characteristics of upstream energetic (E≥50 keV) ion events during intense geomagnetic activity;Journal of Geophysical Research: Space Physics;1998-05-01
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